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On the Production of Meteor Streams by Cometary Nuclei

Published online by Cambridge University Press:  14 August 2015

L. A. Katasev  and
N. V. Kulikova
L. A. Katasev
Affiliation:
Institute for Experimental Meteorology, Obninsk, U.S.S.R.
N. V. Kulikova
Affiliation:
Institute for Experimental Meteorology, Obninsk, U.S.S.R.

Abstract

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An attempt is made to use Monte-Carlo techniques to model the process of formation of meteor streams. It is supposed that meteor streams are formed as the result of ejection of meteoroids from a cometary nucleus at perihelion. Possible ejection velocities are determined for the Draconids, Perseids, Leonids, and Taurids. In general the values do not exceed 100 m s-1. The data obtained can also be used to estimate the ages of the streams.

Type
Part VI/Relationship With Meteors and Minor Planets
Information
Symposium - International Astronomical Union , Volume 45: The Motion, Evolution of Orbits and Origin of Comets , 1972 , pp. 498 - 502
Copyright
Copyright © Reidel 1972 

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